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An Overview of the Second Round of the Mock LISA Data Challenges
Classical and Quantum Gravity
  • K. A. Arnaud
  • S. Babak
  • J. G. Baker
  • M. J. Benacquista
  • N. J. Cornish
  • C. Cutler
  • Shane L. Larson, Utah State University
  • B. S. Sathyaprakash
  • M. Vallisneri
  • A. Vecchio
  • J-Y. Vinet
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The Mock Data Challenges (MLDCs) have the dual purpose of fostering the development of LISA data-analysis tools and capabilities and of demonstrating the technical readiness already achieved by the gravitational-wave community in distilling a rich science payoff from the LISA data. The first round of MLDCs has just been completed and the second-round data sets are being released shortly after this workshop. The second-round data sets contain radiation from an entire Galactic population of stellar-mass binary systems, from massive-black-hole binaries, and from extreme-mass-ratio inspirals. These data sets are designed to capture much of the complexity that is expected in the actual LISA data, and should provide a fairly realistic setting to test advanced data-analysis techniques, and in particular the global aspect of the analysis. Here we describe the second round of MLDCs and provide details about its implementation.


Originally published by Institute of Physics in Classical and Quantum Gravity. Publisher's PDF available through remote link. May require subscription if user is not on the USU Network.
Citation Information
An overview of the second round of the Mock LISA Data Challenges. K. A. Arnaud, S. Babak, J. G. Baker, M. J. Benacquista, N. J. Cornish, C. Cutler, S. L. Larson, B. S. Sathyaprakash, M. Vallisneri, A. Vecchio, J-Y. Vinet (The Mock LISA Data Challenge Task Force). Classical & Quantum Gravity 24, S551-564 (2007).